J/A+AS/125/219ivo://CDS.VizieR/J/A+AS/125/219CDSAdelman S.J.Pintado O.I.2000-01-19T19:56:05Z2000-01-19T20:55:47ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frpeculiar-variable-starschemical-abundancesElemental abundances are derived for four sharp-lined stars, the Mercury-Manganese stars {mu} Lep, HR 4817, and 28 Her, and 7 Sex, a Population I star with Population II space motions, using REOSC echelle spectrograms obtained at CASLEO to extend previous studies. Comparisons with published equivalent widths indicate that the CASLEO scale is marginally larger than those of DAO Reticon and KPNO CCD spectra. The CASLEO spectrograms have improved the quality of the abundance determinations. New abundances are found for a few elements.1997A&AS..125..219Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/125/219CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994)J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)J/A+AS/137/227 : HD 133029 & HD 192913 abundances (Lopez-Garcia+ 1999)J/A+A/354/899 : Elemental abundance analyses, IV. (Adelman+, 2000)J/MNRAS/316/514 : 28 And & 99 Her elemental abundances (Adelman+, 2000)J/A+A/367/597 : ups Her, phi Her & HR 7018 abundances (Adelman+, 2001)J/A+A/367/859 : {alpha} Scl and HD 170973 abundances (Lopez-Garcia+, 2001)J/A+A/394/187 : {gamma} Ser & 101 Her elemental abundances (Caliskan+, 2002)J/A+A/406/975 : theta And, eps Del, eps Aqr, iota And (Kocer+, 2003)J/A+A/406/987 : xi Oct, alpha Sex, 68 Tau elemental abund. (Pintado+, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/125/219https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/125/219http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/125/219https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/125/219https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/125/219http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/125/219GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+AS/125/219/abundAtomic abundances (table3 to table6)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharIonIonphys.atmol.ionizationcharprimaryNlineNumber of linesmeta.numberintElementElement (identical to bytes 9-10)phys.atmol.elementcharl_log(Nel/Ntot)Limit flag on log(Nel/Ntot)meta.code.errorcharlog(Nel/Ntot)Derived abundance of Element (ratio of number of atoms to the total number of atoms per unit volume)phys.abundfloate_log(Nel/Ntot)? rms uncertainty on log(Nel/Ntot)stat.errorfloatnullableu_e_log(Nel/Ntot)Uncertainty flag on e_log(Nel/Ntot)meta.code.errorcharJ/A+AS/125/219/newlinesNew lines (table3 to table6)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharIonIonphys.atmol.ionizationcharprimaryMult? Multiplet numberphys.atmol.levelcharlambdaWavelength0.1nmem.wlfloatlog(gf)log(gf) valuephys.atmol.wOscStrengthfloatr_log(gf)Reference for log(gf) (1)meta.refcharEWEquivalent width0.0001nmspect.line.eqWidthintlog(N/Ntot)Derived abundance in relative number of atomsphys.abundfloat